The file "herschel-bat-photometry.csv" contains Herschel PACS and SPIRE photometry
for the Herschel-BAT sample. The file contains 1 row for each of the 313 sources that
were imaged in our Herschel survey as well as a header row with names for the columns.
There are 14 columns with the following data contained in them:

Column 1: Name of the Swift/BAT AGN
Column 2: PACS 70 micron flux in Jy. If value is 0, then only a 5-sigma upper limit was measured
          for this source and is contained in next column.
Column 3: PACS 70 micron 1-sigma error OR 5-sigma upper limit
Column 4: PACS 160 micron flux in Jy. If value is 0, then only a 5-sigma upper limit was measured
          for this source and is contained in next column.
Column 5: PACS 160 micron 1-sigma error OR 5-sigma upper limit
Column 6: SPIRE 250 micron flux in Jy. If value is 0, then only a 5-sigma upper limit was measured
          for this source and is contained in next column.
Column 7: SPIRE 250 micron 1-sigma error OR 5-sigma upper limit
Column 8: SPIRE 250 micron flag. Flag values are as follows:
          A: Source was cleanly detected above 5-sigma
          U: Source is undetected at the 5-sigma level
          The following flags can be added onto an "A" or "U":
          C: Image is likely contaminated by foreground cirrus
          d: There is a nearby companion source to the AGN but unlikely to be affecting
             the photometry significantly.
          D: There is a nearby companion source to the AGN that is likely to be affecting
             the photometry significantly.
Column 9: SPIRE 350 micron flux in Jy. If value is 0, then only a 5-sigma upper limit was measured
          for this source and is contained in next column.
Column 10: SPIRE 350 micron 1-sigma error OR 5-sigma upper limit
Column 11: SPIRE 350 micron flag. Flag values are as follows:
          A: Source was cleanly detected above 5-sigma
          U: Source is undetected at the 5-sigma level
          The following flags can be added onto an "A" or "U":
          C: Image is likely contaminated by foreground cirrus
          d: There is a nearby companion source to the AGN but unlikely to be affecting
             the photometry significantly.
          D: There is a nearby companion source to the AGN that is likely to be affecting
             the photometry significantly.
Column 12: SPIRE 500 micron flux in Jy. If value is 0, then only a 5-sigma upper limit was measured
          for this source and is contained in next column.
Column 13: SPIRE 500 micron 1-sigma error OR 5-sigma upper limit
Column 14: SPIRE 500 micron flag. Flag values are as follows:
          A: Source was cleanly detected above 5-sigma
          U: Source is undetected at the 5-sigma level
          The following flags can be added onto an "A" or "U":
          C: Image is likely contaminated by foreground cirrus
          d: There is a nearby companion source to the AGN but unlikely to be affecting
             the photometry significantly.
          D: There is a nearby companion source to the AGN that is likely to be affecting
             the photometry significantly.